Published August 1985 | Version v1
Report

New calorimetric all-particle energy spectrum

Creators

Description

Both the maximum size N sub m and the sea level muon size N sub mu have been used separately to find the all-particle energy spectrum in the air shower domain. However the conversion required, whether from N sub m to E or from N sub mu to E, has customarily been carried out by means of calculations based on an assumed cascase model. It is shown here that by combining present data on N sub m and N sub mu spectra with data on: (1); the energy spectrum of air shower muons and (2) the average width of the electron profile, one can obtain empirical values of the N sub m to E and N sub mu to E conversion factors, and an empirical calorimetric all-particle spectrum, in the energy range 2 x 10 to the 6th power E 2 x 10 to the 9th power GeV

Additional details

Publishing Information

Imprint Title
Ninteenth International Cosmic Ray Conference. OG sessions, volume 2
Journal Page Range
vp.
Report number
NASA-CP--2376-VOL-2

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
17080796
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Non-conventional Literature
Descriptors DEI
COSMIC ELECTRONS; COSMIC MUONS; COSMIC NEUTRINOS; COSMIC SHOWERS; ENERGY SPECTRA; NUCLEONS
Descriptors DEC
BARYONS; COSMIC RADIATION; ELECTRONS; ELEMENTARY PARTICLES; FERMIONS; HADRONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MUONS; NEUTRINOS; RADIATIONS; SECONDARY COSMIC RADIATION; SHOWERS; SPECTRA